Volcanic activity, or volcanism, has played a significant role in the geologic evolution of Mars.[2] Scientists have known since the Mariner 9 mission in 1972 that volcanic features cover large portions of the Martian surface. These features include extensive lava flows, vast lava plains, and, such as Olympus Mons, the largest known volcanoes in the Solar System.[3][4] Martian volcanic features range in age from Noachian (>3.7 billion years) to late Amazonian (< 500 million years), indicating that the planet has been volcanically active throughout its history,[5] and some speculate it probably still is so today.[6][7][8] Both Mars and Earth are large, differentiatedplanets built from similar chondritic materials.[9] Many of the same magmatic processes that occur on Earth also occurred on Mars, and both planets are similar enough compositionally that the same names can be applied to their igneous rocks.
^"History". www.jpl.nasa.gov. Archived from the original on 3 June 2016. Retrieved 3 May 2018.
^Head, J.W. (2007). The Geology of Mars: New Insights and Outstanding Questions in The Geology of Mars: Evidence from Earth-Based Analogs, Chapman, M., Ed; Cambridge University Press: Cambridge UK, p. 10.
^"Hunting for young lava flows". Geophysical Research Letters. Red Planet. 1 June 2011. Archived from the original on 4 October 2013. Retrieved 4 October 2013.